Radek Poleski
Radek Poleski
Function `solve()` returns more output. Then there is no need to re-read the file to run e.g., `Analyzer.get_data()`.
I'm writing code for cleaning the data. It involves masking and un-masking points as bad. I've found it quite complicated - one cannot do ```python dataset.bad[i] = True ``` because...
In example 16 it would be good to have option to include the burn-in on the trace plot (and no other plots). In that case, the burn-in should be on...
Can someone make a logo for MulensModel project? The image below is from @justi. I like the model and the lens. Something that could be changed is the peak of...
It's time to add astrometric microlensing to MM. Recently @skterry approached me and asked for it. We should start with **use cases - can somebody draft them?** We should think...
While pringing ModelParameters with parallax, we should get e.g.: ``` t_0 (HJD) u_0 t_E (d) pi_E_N pi_E_E 2456789.01235 0.123000 123.0000 0.45600 0.12300 t_0_par = 2457000.00000 ``` or ``` t_0 (HJD)...
```python >>> import MulensModel as mm >>> params = mm.ModelParameters({'t_0': 0, 'u_0': 1., 't_E': 9., 's': 1.5, 'q': 0.5, 'alpha': 90.}) >>> mag_curve = mm.MagnificationCurve([0, 1., 10.], params) >>> mag_curve.get_magnification()...
@jenniferyee recently made this commit: 6836cbd646fbb02a252a15368f5db9b04b86cbbe. I've found it complicated and thought how to simplify this code. First, it seems impossible to have `self.fix_source_flux` of *float* type, because `__init__` says:...
What is decided to be done for Version 3: - [x] derivatives of magnification and complicated structure of PointLens - architecture changes are made by @jenniferyee in [Version3_1 branch](https://github.com/rpoleski/MulensModel/compare/master...Version3_1); #107...
We have interpolation for elliptical integrals in `pointlens.py` for WM94. These grid of elliptical integral of the 3rd kind was set to get relative accuracy of 10^-4. Based on a...